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Accurate mass and radius determinations of a cool subdwarf in an eclipsing binary

Cool subdwarfs are metal-poor low-mass stars that formed during the early stages of the evolution of our Galaxy. Because they are relatively rare in the vicinity of the Sun, we know of few cool subdwarfs in the solar neighbourhood, and none with both the mass and the radius accurately determined. Th...

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Detalhes bibliográficos
Publicado no:Nat Astron
Main Authors: Rebassa-Mansergas, Alberto, Parsons, Steven G., Dhillon, Vikram S., Ren, Juanjuan, Littlefair, Stuart P., Marsh, Thomas R., Torres, Santiago
Formato: Artigo
Idioma:Inglês
Publicado em: 2019
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Acesso em linha:https://ncbi.nlm.nih.gov/pmc/articles/PMC6558239/
https://ncbi.nlm.nih.gov/pubmed/31187071
https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1038/s41550-019-0746-7
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